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Lucas - WordPress.com
Lucas - WordPress.com

... Hydra, the sea serpent, with it’s long, serpentine shape, is the largest constellation by area, in the sky. Hydra is sandwiched between the plane of the Solar System (the ecliptic) to the north, and the plane of the Milky Way galaxy to the south. Just out of reach of the galactic plane, there aren’t ...
Lecture 20: Formation of Planets, Exoplanets 3/30
Lecture 20: Formation of Planets, Exoplanets 3/30

... PHYS 162 life ...
The Dynamics-Based Approach to Studying Terrestrial Exoplanets
The Dynamics-Based Approach to Studying Terrestrial Exoplanets

... (Henry et al. 2007) report 348 stars within 10 pc (as determined from trigonometric parallaxes), of which 239 are M dwarfs and only 21 are G dwarfs. Projecting these numbers by volume, we expect 10,000 M-dwarf stars within 35 pc. This estimate is consistent with the number of Mdwarfs in that volume ...
Introduction to Basic Stargazing Part I - Naples Free-Net
Introduction to Basic Stargazing Part I - Naples Free-Net

... Take your star chart and look for the constellation Hercules, just for an example. You will note that the constellation Hercules as drawn does not look much like a man; constellations only occasionally look like the objects they are supposed to represent. The lines are drawn only to serve as a mnemo ...
Exoplanet, 51 Pegasi b, Solar System, VLT, La Silla. ESOcast
Exoplanet, 51 Pegasi b, Solar System, VLT, La Silla. ESOcast

... richest planetary system yet. The system, located over 120 light-years away around the Sun-like star HD 10180, contains at least five exoplanets. There is also tantalising evidence that two more planets may be present in this system, one of which would have the lowest mass ever found. ...
Extrasolar Planetary Systems » American Scientist
Extrasolar Planetary Systems » American Scientist

... The following year, David W. Latham of the Harvard-Smithsonian Center for Astrophysics and four colleagues reported strong evidence for what might be a planet orbiting an obscure star known as HD 114762. Because Latham's planet has at least 10 times the mass of Jupiter, astronomers tended to assume ...
AyC10 Fall 2007: Midterm 2 Review Sheet
AyC10 Fall 2007: Midterm 2 Review Sheet

... What does it mean for a star to be on the Main Sequence? A star is on the Main Sequence when its core is fusing hydrogen into helium. During this phase, stars are mostly stable and obey well-defined relationships between their mass, luminosity, and surface temperature (note: L  M4 only applies to M ...
Gökküre
Gökküre

... wants to reach the greatest fire (the Sun), the bubbles in water rise up because air is to be above water, etc. ...
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ppt

... days for both RV and transit discovered planets. 5. Most transiting giant planets have densities near that of Saturn. It is not known if this is due to their close proximity to the star (i.e. inflated radius) 6. Transiting planets have been discovered around stars fainter than those from radial velo ...
ph709-09
ph709-09

... et al. 2006; Ikoma et al. 2006). Understanding how the transiting planet massradius relations change as a function of orbital distance, stellar mass, stellar metallicity, or UV flux, will provide insight into the fundamentals of planetary formation, migration, and evolution. The transit method of pl ...
Supernova - Mid-Pacific Institute
Supernova - Mid-Pacific Institute

...  The core is crushed into a tiny object called a neutron star, which may be no more than 6 mi (10 ...
The Kepler spacecraft has found thousands of likely extrasolar
The Kepler spacecraft has found thousands of likely extrasolar

... ust over 20 years ago, astronomers first detected signs of planets outside our solar system. Initially, they expected to find solar systems like ours, but they quickly realized that isn’t how nature works. In fact, one of the first exoplanets discovered is about Jupiter’s mass but circles its Sun-li ...
Light of Distant Stars - Glasgow Science Centre
Light of Distant Stars - Glasgow Science Centre

... Jeremiah Horrocks was an English astronomer who lived in the 17th century. He wrote about the first observed transit of Venus. Here is his account of the event, as taken from his book Venus in Sole Visa: When the time of the observation approached, I retired to my apartment, and having closed the wi ...
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- Europhysics News

... The huge diversity in the physical and orbital properties of exoplanets forces us to reconsider the model of planetary formation currently accepted for the solar system. This model is based upon the properties of planetary orbits, mostly coplanar, circular and concentric around the Sun. Following th ...
The 22 First Magnitude Stars
The 22 First Magnitude Stars

... Flamsteed Numbers • Number + genitive of constellation name (e.g., 66 Geminorum) • Assigned to stars from west to east • Greek Bayer letters usually take precedence ...
Comets and Asteroids Up-close
Comets and Asteroids Up-close

... Ceres: Dwarf planet Ceres is the largest object in the asteroid belt between Mars and Jupiter and the only dwarf planet located in the inner solar system. It was the first member of the asteroid belt to be discovered when Giuseppe Piazzi spotted it in 1801. ...
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... Continuing Bombardment of the Planets • Although the crater is completely covered by sediments, mineral samples show that it contains shocked quartz typical of impact sites and that it is the right age. ...
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... D. Its smaller size means it has gravitational attraction that is too weak to hold onto an atmosphere. 13. Which terrestrial planet has the most moons? A. Mercury B. Venus C. Earth D. Mars 14. Besides the Earth, which terrestrial planet also has seasons? A. Mercury B. Venus C. Mars D. Seasons are un ...
Beyond Pluto
Beyond Pluto

... PLANETS lack a standard definition. If a body orbits a sun and was made spherical by its own gravity, astronomers tend to call it a planet. Yet that definition would include at least four asteroids and dozens of Kuiper belt objects. ASTEROIDS (a.k.a. minor planets) are rocky, metallic, or carbonaceo ...
Oct - Seattle Astronomical Society
Oct - Seattle Astronomical Society

... Eris will be at opposition, and closest to the Earth at a mere 95.778 AU, on October 14, and will certainly be observed by several of the largest telescopes. I was able to participate in a teleconference with Brown, and I asked him about the status of TNO observations. He said that a number of findi ...
The Night Sky
The Night Sky

... Every August, the night sky produces its own version of fireworks, the Perseid meteor shower. This meteor shower is a summertime classic and among the oldest and most publicized of all such showers. Astronomers have determined that comet Swift-Tuttle is the source of the Perseid shower as once every ...
SPECIAL REPORT
SPECIAL REPORT

... struck the early Earth off-center. This created a spray of debris trapped in Earth orbit that later accreted to form the Moon. Detailed models of these processes give astronomers a reasonably complete picture of how terrestrial planets formed. Planetbuilding appears to be an intrinsically chaotic pr ...
ph507-16-1exo2
ph507-16-1exo2

... Using high-contrast, near-infrared adaptive optics observations with the Keck and Gemini telescopes, the team of researchers were able to see three orbiting planetary companions to HR8799 ...
Phys 214. Planets and Life
Phys 214. Planets and Life

... Many brown dwarfs in constellation Orion. Infrared image of a Jupiter-size planet orbiting a brown dwarf. Brown dwarfs are substellar objects with insufficient mass to sustain nuclear fusion in their cores. They have higher surface temperatures than planets and masses between 10to 80 times that of J ...
Solar System
Solar System

... 5. The orbits of all the planets lie in a flat plane except for the orbit of Pluto (dwarf planet, which is tilted compared to the other orbits. 6. Mercury and Venus are the only two planets that do not have at least one moon. 7. Mars looks like a red star in the sky. 8. Jupiter has a striped appeara ...
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Astronomical naming conventions

In ancient times, only the Sun and Moon, a few hundred stars and the most easily visible planets had names. Over the last few hundred years, the number of identified astronomical objects has risen from hundreds to over a billion, and more are discovered every year. Astronomers need to be able to assign systematic designations to unambiguously identify all of these objects, and at the same time give names to the most interesting objects and, where relevant, features of those objects.The International Astronomical Union (IAU) is the officially recognized authority in astronomy for assigning designations to celestial bodies such as stars, planets, and minor planets, including any surface features on them. In response to the need for unambiguous names for astronomical objects, it has created a number of systematic naming systems for objects of various sorts.
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